| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.80 | 145.32 | 51.84 | 233.50 | -14.47 | 116.42 | -69.32 | 107.60 | 0.9508 | 121.1 | -99.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.62 | 28.63 | 14.50 | 39.61 | -14.05 | 119.64 | -66.10 | 107.86 | 0.9334 | 607.7 | -38.8 | |
| 0.00 | 1.23 | 0.00 | 1.73 | -14.22 | 119.00 | -66.74 | 107.88 | 0.9373 | 174.0 | 113.4 | |
| 7.29 | 20.99 | 10.30 | 30.17 | -13.89 | 118.79 | -66.95 | 107.50 | 0.9381 | 514.9 | 208.8 | |
| 0.00 | 6.76 | 0.00 | 9.57 | -13.43 | 118.66 | -67.08 | 106.99 | 0.9383 | 424.0 | 371.5 | |
| 0.00 | 0.88 | 0.00 | 1.29 | -14.13 | 118.08 | -67.66 | 107.58 | 0.9424 | -354.0 | -317.6 | |
| 1.76 | -3.00 | 2.56 | -3.00 | -13.91 | 118.05 | -67.69 | 107.35 | 0.9423 | 266.3 | 999999 | |
| 2.72 | 33.10 | 4.21 | 50.85 | -14.87 | 117.09 | -68.65 | 108.13 | 0.9486 | -720.9 | -545.4 | |
| 0.61 | -7.00 | 0.95 | -7.00 | -14.64 | 117.16 | -68.58 | 107.91 | 0.9480 | -672.0 | 999999 | |
| 0.00 | 1.14 | 0.00 | 1.71 | -13.51 | 117.38 | -68.36 | 106.79 | 0.9455 | 156.0 | 131.5 | |
| 1.93 | 2.28 | 2.96 | 3.50 | -13.64 | 117.04 | -68.70 | 106.85 | 0.9475 | -89.3 | -102.0 | |
| 1.76 | 3.86 | 3.00 | 6.61 | -15.51 | 115.26 | -70.47 | 108.40 | 0.9584 | -189.6 | -58.3 | |
| 0.00 | 1.58 | 0.00 | 2.50 | -13.68 | 116.40 | -69.33 | 106.76 | 0.9508 | 169.0 | 55.6 | |
| 1.84 | 44.87 | 3.36 | 85.96 | -15.07 | 114.06 | -71.68 | 107.71 | 0.9635 | -190.1 | 11.5 | |
| 5.27 | -13.00 | 10.00 | -13.00 | -14.69 | 113.26 | -72.48 | 107.16 | 0.9666 | -333.9 | 999999 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |